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  Why can soft X-Ray transients remain in the low/hard state during outburst

Meyer-Hofmeister, E. (2004). Why can soft X-Ray transients remain in the low/hard state during outburst.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0011-B7E6-0 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0011-B7E7-E
Genre: Conference Paper

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 Creators:
Meyer-Hofmeister, E.1, 2, Author              
Affiliations:
1Stellar Astrophysics, MPI for Astrophysics, Max Planck Society, ou_159882              
2High Energy Astrophysics, MPI for Astrophysics, Max Planck Society, ou_159881              

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Language(s):
 Dates: 2004
 Publication Status: Published in print
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Method: -
 Identifiers: eDoc: 206737
URI: http://ptp.ipap.jp/link?PTPS/155/383
Other: Reihe: Progress....
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Title: Stellar-mass, intermediate-mas, and supermassive black holes
Place of Event: Kyoto, Japan
Start-/End Date: 2003-10-28 - 2003-10-31

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Title: Stellar-mass, intermediate-mass, and supermassive black holes
Source Genre: Issue
 Creator(s):
Mineshige, Shin, Editor
Makishima, Kazuo, Editor
Affiliations:
-
Publ. Info: -
Pages: - Volume / Issue: - Sequence Number: - Start / End Page: 383 - 384 Identifier: -

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Title: Progress of Theoretical Physics, Supplement
  Alternative Title : Prog. theor. phy. suppl.
Source Genre: Journal
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Publ. Info: -
Pages: - Volume / Issue: (155) Sequence Number: - Start / End Page: - Identifier: ISSN: 0375-9687